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Structure of the electromagnetic fields of loop radiators in magnetized plasmas over the whistler frequency range

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Abstract

The role of different sections of the spatial spectrum of whistler waves excited by a loop antenna in the formation of an electromagnetic field structure is investigated experimentally and theoretically. Primary attention is given to the intermediate range of distances between the source and the observation point.

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Authors and Affiliations

  1. Radiophysical Research Institute and Institute of Applied Physics of the Russian Academy of Sciences, Nizhny Novgorod

    T. M. Zaboronkova, A. V. Kostrov, A. V. Kudrin, A. I. Smirnov & A. A. Shaikin

Authors
  1. T. M. Zaboronkova
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  2. A. V. Kostrov
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  3. A. V. Kudrin
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  4. A. I. Smirnov
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  5. A. A. Shaikin
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 39, No. 2, pp. 192–202, February, 1996.

T. M. Zaboronkova, A. V. Kostrov, A. I. Smirnov, and A. A. Shaikin are grateful to The Russian Foundation for Fundamental Research (Grant No.94-02-05447a) and the George Soros International Foundation (Grant No. NOP 300) for financial support. A. V. Kudrin is grateful to the Russian Fund for Fundamental Research (Grant No. 96-02-18666) for financial support.

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Zaboronkova, T.M., Kostrov, A.V., Kudrin, A.V. et al. Structure of the electromagnetic fields of loop radiators in magnetized plasmas over the whistler frequency range. Radiophys Quantum Electron 39, 132–139 (1996). https://doi.org/10.1007/BF02275367

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  • DOI: https://doi.org/10.1007/BF02275367

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